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Title: |
Numerical Modeling of Space Plasma Flows, Astronum-2009
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Volume: |
429
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Year: |
2010
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View this Volume on ADS
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Editors: |
Pogorelov, Nikolai V.; Audit, Edouard; Zank, Gary P.
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Synopsis: |
This Volume contains the proceedings of ASTRONUM-2009 — the fourth in a series of international conferences now organized by the Center for Space Plasma and Aeronomic Research at the University of Alabama in Huntsville and the Laboratory for Research into the Fundamental Laws of the Universe at the French Commissariat of Atomic Energy. The subjects of the conference included such topics as turbulence and cosmic ray transport, astrophysical flows, space plasma flows, kinetic and hybrid simulations, numerical methods, algorithms, and frameworks, and data handling and visualization. All of these topics are of great importance for scientists investigating solar structure, the heliosphere, the Sun-Earth connection, and various astrophysical phenomena.
The problems discussed at the conference are characterized by different time and space scales, regions, or particle populations, for which different sets of defning equations or concepts are necessary to understand the physical system in its entirety. This book will be of interest to specialists in applied mathematics, astrophysics, space physics, and computer science working on the application of novel numerical algorithms to contemporary problems arising in these fields. It can also be used by graduate students to get acquainted with the fundamental approaches to solving the fluid dynamic and kinetic equations governing space plasma flows.
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ISBN: |
978-1-58381-738-4
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eISBN:
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978-1-58381-739-1
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Paper Title |
Page |
Authors |
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Volume Cover |
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Pogolorov, N. P.; Audit, E.; Zank, G. P. |
Front Matter |
1 |
Pogolorov, N. P.; Audit, E.; Zank, G. P. |
Part I. Turbulence and Cosmic Ray Transport |
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Non-ideal MHD Turbulent Decay in Molecular Clouds |
3 |
Downes, T. P.; O’Sullivan, S. |
Supersonically Turbulent, Shock Bound Interaction Zones |
9 |
Folini, D.; Walder, R.; Favre, J. M. |
Self-organization in Turbulent Molecular Clouds: Compressional Versus Solenoidal Modes |
15 |
Kritsuk, A. G.; Ustyugov, S. D.; Norman, M. L.; Padoan, P. |
Star Formation in a Turbulent Cloud Core with Self-gravitational MHD Adaptive Mesh Refinement |
22 |
Matsumoto, T. |
Understanding Nonlinear Cascades in Magnetohydrodynamic Turbulence by Statistical Closure Theory |
28 |
Müller, W.; Malapaka, S. K. |
Relativistic Particle Acceleration in Tangled Magnetic Fields |
33 |
O’Sullivan, S.; Reville, B.; Taylor, A.; Taylor, A. |
Turbulence and Magnetic Fields in the Intergalactic Medium of
the Universe |
39 |
Ryu, D.; Kang, H.; Cho, J. |
Alfvénic Turbulence Simulation in a Realistic Solar Wind |
51 |
Usmanov, A. V.; Goldstein, M. L. |
Part II. Astrophysical Flows |
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Structure and Fragmentation of Turbulent Interstellar Clouds |
59 |
Audit, E.; Hennebelle, P. |
Radiation-Magneto-Hydrodynamics Calculations of a Dense Core Collapse |
66 |
Commerçon, B.; Hennebelle, P.; Audit, E.; Chabrier, G.; Teyssier, R. |
Relativistic MHD Simulations of Alfvén QPOs in Magnetars |
72 |
Font, J. A.; Cerdá -Durán, P.; Stegioulas, N. |
Large- and Small-Scale Dynamo Action |
79 |
Hughes, D. W. |
Self-Similar Evolution of Cosmic-Ray Modified Shocks |
85 |
Kang, H.; Ryu, D. |
Relativistic Hydro and Magnetohydrodynamic Models for AGN Jet Propagation and Deceleration |
91 |
Keppens, R.; Meliani, Z. |
Feedback Effects in the High Mass and Low Mass Star Formation |
97 |
Klein, R. I. |
An Approach to the Riemann Problem for SPH Inviscid Ideal Flows: Consequences for the Equation of State |
106 |
Lanzafame, G. |
Reconnection Diffusion and Star Formation Processes |
113 |
Lazarian, A.; Santos-Lima, R.; de Gouveia Dal Pino, E. |
Relativistic Two-component Jet Evolutions in 2D and 3D |
121 |
Meliani, Z.; Keppens, R. |
Simulation of Relativistic Shocks and Associated Radiation |
127 |
Nishikawa, K.; Niemiec, J.; Medvedev, M.; Zhang, B.; Hardee, P.; Mizuno, Y.; Nordlund, A.; Frederiksen, J.; Sol, H.; Pohl, M.; Hartmann, D. H.; Oka, M.; Fishman, J. F. |
Simulations of the Magneto-rotational Instability in Core-Collapse Supernovae |
136 |
Obergaulinger, M.; Cerdá -Durán, P.; Müller, E.; Aloy, M. A. |
Modeling the Diversity of Type Ia Supernova Explosions |
142 |
Röpke, F. K.; Hillebrandt, W.; Kasen, D.; Woosley, S. E. |
Monte Carlo Radiative Transfer Simulations: Applications to Astrophysical Outflows and Explosions |
148 |
Sim, S. A.; Kromer, M.; Röpke, F. K.; Sorokina, E. I.; Blinnikov, S. I.; Kasen, D.; Hillebrandt, W. |
A Galaxy in the Making |
154 |
Slyz, A.; Devriendt, J.; Powell, L. |
A Numerical Model for Multigroup Radiation Hydrodynamics |
160 |
Vaytet, N.; Audit, E.; Dubroca, B. |
Implicit Hydrodynamic Simulations of Stellar Interiors |
167 |
Viallet, M.; Baraffe, I.; Mulet-Marquis, C.; Lévêque, E.; Walder, R.; Freytag, B.; Winisdoerffer, C. |
Recurrent Novae: Progenitors of SN Ia? |
173 |
Walder, R.; Folini, D.; Favre, J. M.; Shore, S. N. |
Part III. Space Plasma Flows |
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Small-scale Dynamo Action in Compressible Convection |
181 |
Bushby, P. J.; Proctor, M. R. E.; Weiss, N. O. |
Physics of Thrust Prediction of the Solar Wind Electric Sail Propulsion System |
187 |
Janhunen, P. |
Grid Convergence of the HYB-Venus Hybrid Simulation |
193 |
Jarvinen, R.; Kallio, E.; Janhunen, P.; Pohjola, V.; Sillanpää, I. |
Three-Dimensional Simulations of the Parker’s Model of Solar Coronal Heating: Lundquist Number Scaling due to Random Photospheric Footpoint Motion |
201 |
Ng, C. S.; Lin, L.; Bhattacharjee, A. |
4D Model for the Solar Environment |
207 |
Oran, R.; Sokolov, I. V.; Roussev, I. I.; Van Der Holst, B.; Manchester, W. B.; Gombosi, T. I. |
Multi-Ion Magnetohydrodynamics |
213 |
Toth, G.; Glocer, A.; Ma, Y.; Najib, D.; Gombosi, T. |
Breakout Coronal Mass Ejection or Streamer Blowout: the Bugle Effect |
219 |
van der Holst, B. |
Part IV. Kinetic and Hybrid Simulations |
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Kinetic Modeling of Interstellar Hydrogen in the Heliosphere |
227 |
Heerikhuisen, J.; Pogorelov, N. V. |
The Kinetic Approach to Model Space Plasmas |
233 |
Pierrard, V. |
Part V. Numerical Methods, Algorithms, and Frameworks |
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A New Scheme to Solve Gas Disks around Stars |
241 |
Hanawa, T. |
Exploiting the Extensibility of the FLASH Code Architecture for Unsplit Time Integration |
247 |
Lee, D.; Dubey, A.; Olson, K.; Weide, K.; Antypas, K. |
(Semi-)Analytical Solutions of 1D Partial Differential Equations |
253 |
Lesaffre, P. |
High Order Finite Difference Schemes for MHD |
258 |
Mignone, A.; Tzeferacos, P. |
Modeling Heliospheric Phenomena with the Multi-Scale Fluid-Kinetic Simulation Suite |
266 |
Pogorelov, N. V.; Borovikov, S. N.; Heerikhuisen, J.; Kryukov, I. A.; Zank, G. P. |
Smoothed Particle Hydrodynamics: Turbulence and MHD |
274 |
Price, D. J.; Federrath, C. |
ADER Schemes for Time-Dependent PDEs: Review and Applications to Astrophysics |
281 |
Toro, E. F.; Dumbser, M. |
Characteristic Boundary Conditions for Numerical Magnetohydrodynamic (MHD) Simulation of Solar and Laboratory Plasma Flows |
294 |
Wu, S. T.; Wang, A. H.; Cassibry, J. |
Part VI. Data Handling and Visualization |
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The Virtual Model Repository (VMR) |
305 |
De Zeeuw, D. L.; Ridley, A. J.; Bashkirov, V. |
Visualizing the Reionization of the Universe on Programmable Graphics Hardware |
311 |
Kaehler, R.; Alvarez, M.; Abel, T. |
PRACE: Partnership for Advanced Computing in Europe Preparation of a Petascale Supercomputing Infrastructure for European Scientists |
317 |
Turunen, A.; Nominé , J.-P.; Robin, F.; Erwin, D.; Huber, H.; Berg, A.; Murri, R.; Simpson, A. |
VAPOR: Visual, Statistical, and Structural Analysis of Astrophysical Flows |
323 |
Clyne, J.; Gruchalla, K.; Rast, M. |
Recent Advances in VisIt: AMR Streamlines and Query-driven Visualization |
329 |
Weber, G. H.; Ahern, S.; Bethel, E. W.; Borovikov, S.; Childs, H. R.; Deines, E.; Garth, C.; Hagen, H.; Hamann, B.; Joy, K. I.; Martin, D.; Meredith, J.; Prabhat; Pugmire, D.; Rübel, O.; Van Straalen, B.; Wu, K. |
Back Matter |
335 |
Pogolorov, N. P.; Audit, E.; Zank, G. P. |
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